4th CRISM conference

Cosmic Rays and the InterStellar Medium

25 - 29 June 2018
Grenoble (France)

Friday 29
CR transport in the ISM: role of self-generated turbulence, large-scale injected turbulence, direct and indirect observations, modelling and phenomenology, link to dark matter detection
Gloria Dubner
› 11:00 - 11:25 (25min)
Galactic Magnetic field from polarized emission at CMB frequencies
Vincent Pelgrims  1@  
1 : Laboratoire de Physique Subatomique et Cosmologie  (LPSC - Grenoble)  -  Website
LPSC - Grenoble
53 Avenue des Martyrs 38026 Grenoble Cedex -  France

Galactic magnetic field manifests itself through a large variety of physical phenomena. It plays a crucial role in the cosmic ray propagation. Connecting the local and the large-scale Galactic magnetic field might help understanding the ISM physics.In this talk I will review state-of-the-art modeling of the large-scale Galactic magnetic field as inferred from the polarized diffuse emission measured by Planck at radio to sub-mm wavelengths.

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